Structured dispersive sub-keV ions inside the ring current region, or so-called wedge-like dispersions, those which have been considered signatures of long-time drift by ExB and grad-|B| drifts from nightside, are surveyed using the Viking, Freja, Munin, and Cluster satellites. While the ordinary wedge-like dispersion (increasing energy with increasing latitude) is observed mainly in the morning sector at all altitudes (by all spacecrafts), the reversed wedge-like dispersion (decreasing energy with increasing latitude) is observed at different local times by different spacecrafts. The differences between spacecrafts are also found in the H+/O+ ratio and in observation frequency. The observed altitudinal difference indicates that the evolution of drifting particles depends strongly on the mass and mirror altitude.